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Arrayed waveguide gratings for astronomy with multiple offaxis fibre launch

机译:带有多个离轴光纤发射的天文学阵列波导光栅

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The next generation of major ground-based optical and near-infrared astronomical telescopes are planned to have aperture sizes from 25–42 meters in diameter, making them substantially larger than existing telescopes. This has a major impact on seeing limited spectroscopic instrumentation, as the size of the instrument grows in proportion to the telescope aperture for traditional designs and more importantly, the cost of the instrument increases with the telescope aperture squared, or faster [1]. This unsustainable trend has necessitated a miniaturization of devices for astronomy, with integrated photonics showing great promise. Particularly of interest is the integrated photonic spectrograph (IPS) [1,2].
机译:下一代大型地面光学和近红外天文望远镜计划具有25-42米的孔径,使其比现有望远镜大得多。这对于看到有限的光谱仪器会产生重大影响,因为对于传统设计而言,仪器的尺寸与望远镜的孔径成正比增长,更重要的是,仪器的成本随着望远镜孔径的平方或更快而增加[1]。这种不可持续的趋势已使天文学的设备小型化,而集成光子技术显示出巨大的希望。尤其值得关注的是集成光子光谱仪(IPS)[1,2]。

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